BLITS

{{Short description|Russian passive spherical reflector satellite}}

{{other uses}}

{{Infobox spaceflight

| name = BLITS

| image = BLITS 300c target.gif

| image_size = 220

| image_caption = An artist's impression of BLITS

| mission_type = Technology

| operator = Roskosmos
ILRS network

| website =

| COSPAR_ID = 2009-049G

| SATCAT = 35871

| mission_duration = Achieved: 3.5 years
Planned: 5 years

| spacecraft_bus =

| manufacturer = FSUE-IPIE

| launch_mass = {{convert|7.53|kg|lb}}

| dimensions =

| power =

| launch_date = {{start-date|17 September 2009, 15:55:07|timezone=yes}} UTC{{cite web|title=BLITS|url=http://ilrs.gsfc.nasa.gov/missions/satellite_missions/current_missions/blit_general.html|publisher=International Laser Ranging Service|access-date=2014-02-25|archive-url=https://web.archive.org/web/20131017012026/http://ilrs.gsfc.nasa.gov/missions/satellite_missions/current_missions/blit_general.html|archive-date=2013-10-17|url-status=dead}}

| launch_rocket = Soyuz-2-1b/Fregat

| launch_site = Baikonur Site 31/6

| launch_contractor =

| last_contact = March–April 2013

| decay_date =

| orbit_epoch = 25 February 2014, 08:51:29 UTC{{cite web|url=http://www.n2yo.com/satellite/?s=35871|title=BLITS Satellite details 2009-049G NORAD 35871|work=N2YO|date=25 February 2014|access-date=26 February 2014}}

| orbit_reference = Geocentric

| orbit_regime = Low Earth

| orbit_periapsis = {{convert|823|km|mi}}

| orbit_apoapsis = {{convert|829|km|mi}}

| orbit_inclination = 98.55 degrees

| orbit_semimajor = {{convert|7197.67|km|mi}}

| orbit_eccentricity = 0.0004373

| orbit_period = 101.28 minutes

| orbit_RAAN = 105.39 degrees

| orbit_arg_periapsis = 71.58 degrees

| apsis = gee

}}

BLITS (Ball Lens In The Space) is a Russian satellite launched on September 17, 2009, as a secondary payload on a Soyuz-2.1b/Fregat, from the Baikonur Cosmodrome in Kazakhstan.

The satellite is totally passive and spherical, and is tracked using satellite laser ranging (SLR) by the International Laser Ranging Service.{{cite journal |last1=Pearlman |first1=M. |last2=Arnold |first2=D. |last3=Davis |first3=M. |last4=Barlier |first4=F. |last5=Biancale |first5=R. |last6=Vasiliev |first6=V. |last7=Ciufolini |first7=I. |last8=Paolozzi |first8=A. |last9=Pavlis |first9=E. C. |last10=Sośnica |first10=K. |last11=Bloßfeld |first11=M. |title=Laser geodetic satellites: a high-accuracy scientific tool |journal=Journal of Geodesy |date=November 2019 |volume=93 |issue=11 |pages=2181–2194 |doi=10.1007/s00190-019-01228-y|bibcode=2019JGeod..93.2181P |s2cid=127408940 }} The design of BLITS is based on the optical Luneburg lens concept. The retroreflector is a multilayer glass sphere; it provides uniform reflection characteristics when viewed within a very wide range of angles, and can provide a cross-section sufficient for observations at low to medium orbit heights. A similar design was already tested on a smaller laser reflector carried on board of the METEOR-3M spacecraft launched on December 10, 2001.{{cite web|title=Spherical Retroreflector with an Extremely Small Target Error: International Experiment in Space

|url=http://cddis.nasa.gov/lw13/docs/papers/target_vasiliev_1m.pdf

|work=13th International Workshop on Laser Ranging. Toward Millimeter Accuracy|publisher=NASA}}

The purpose of the mission was to validate the spherical glass retroreflector satellite concept and obtain SLR (Satellite Laser Ranging) data for solution of scientific problems in geophysics, geodynamics, and relativity. The BLITS allows millimeter and submillimeter accuracy SLR measurements, as its "target error" (uncertainty of reflection center relative to its center of mass) is less than 0.1 mm. An additional advantage is that the Earth's magnetic field does not affect the satellite orbit and spin parameters, unlike retroreflectors incorporated into active satellites. The BLITS allows the most accurate measurements of any SLR satellites, with the same accuracy level as a ground target.{{cite web| url=http://cddis.gsfc.nasa.gov/lw17/docs/presentations/session6/07-kasi_blits.pdf

|title=BLITS: spin parameters and its optical response measured by the Graz 2kHz SLR system}}

The satellite was inserted into an {{cvt|832|km|||}} Sun-synchronous orbit, with an inclination of 98.85º.{{cite journal |last1=Sośnica |first1=Krzysztof |last2=Jäggi |first2=Adrian |last3=Meyer |first3=Ulrich |last4=Thaller |first4=Daniela |last5=Beutler |first5=Gerhard |last6=Arnold |first6=Daniel |last7=Dach |first7=Rolf |title=Time variable Earth's gravity field from SLR satellites |journal=Journal of Geodesy |date=October 2015 |volume=89 |issue=10 |pages=945–960 |doi=10.1007/s00190-015-0825-1|bibcode=2015JGeod..89..945S |doi-access=free }} The satellite was spinning at a spin period of 5.6 seconds around the axis normal to its orbit plane, allowing laser light to be reflected in short bursts because only half of the satellite is covered in a reflective coating. As the satellite is made of glass, minimal in-flight spin slowdown was expected since there were no conducting parts where currents interacting with the Earth magnetic field can be induced.

The expected operative life was at least five years, but the mission was interrupted in 2013 after a collision with space debris.{{cite web |title=Russian BLITS Satellite hit by Space Debris |url=http://www.spaceflight101.net/blits-satellite-collision-january-2013.html |website=Spaceflight101: Space News and Beyond |access-date=16 April 2020 |archive-url=https://archive.today/20161005043844/http://www.spaceflight101.net/blits-satellite-collision-january-2013.html |archive-date=2016-10-05 |date=9 March 2013 |url-status=usurped}}{{cbignore|bot=InternetArchiveBot}}

Structure

File:BLITS Satellite scheme.gif

The satellite consists of two outer hemispheres (radius {{cvt|85.16|mm|||disp=or}}) made of a low-refraction-index glass (n = 1.47) and an inner ball lens (radius {{cvt|53.52|mm|||disp=or}}) made of a high-refraction-index glass (n = 1.76); the two outer hemispheres and the inner ball are glued together, and one of the outer hemispheres is externally coated with a reflective aluminum coating, covered with a protective varnish. The total mass is {{cvt|7.53|kg|||}}.{{cite web|title=BLITS (Ball Lens In The Space)

|url=https://directory.eoportal.org/web/eoportal/satellite-missions/b/blits

|publisher=ESA, Earth Observation portal}}

The satellite was designed for ranging with a green (532 nm) laser. When used for ranging, the phase center is {{cvt|85.16|mm}} behind the sphere center, with a range correction of +{{cvt|196.94|mm}} taking into account the indices of refraction.{{cite web

|url=http://ilrs.gsfc.nasa.gov/missions/satellite_missions/current_missions/blit_support.html

|title=BLITS LRS Mission Support Status

|access-date=2019-03-06

|archive-url=https://web.archive.org/web/20161016072954/http://ilrs.gsfc.nasa.gov/missions/satellite_missions/current_missions/blit_support.html

|archive-date=2016-10-16

|url-status=dead

}} A smaller spherical retroreflector of the same type but 6 cm in diameter was fastened to the Meteor-3M spacecraft and tested during its space flight of 2001–2006.

Collision

In early 2013, the satellite was found to have a new orbit {{cvt|120|m}} lower, a faster spin period of 2.1 seconds, and a different spin axis. The change was traced back to an event that occurred 22 Jan 2013 at 07:57 UTC; data from the United States's Space Surveillance Network showed that within 10 seconds of that time BLITS was close to the predicted path of a fragment of the former Chinese Fengyun-1C satellite, with a relative velocity of {{cvt|9.6|km/s}} between them. The Chinese government destroyed the Fengyun-1C, at an altitude of {{cvt|865|km}}, on 11 Jan 2007 as a test of an anti-satellite missile, leaving 2,300 to 15,000 pieces of debris.

On January 28, 2013, the International Laser Ranging Service announced that a collision happened between BLITS and a space debris fragment. As a result, an abrupt change occurred of the BLITS orbit parameters (a decrease of the orbiting period), and the spin period changed from 5.6 s before collision to 2.1 s after collision. On April 19, 2013, BLITS mission contacts from the Scientific Research Institute for Precision Instrument Engineering in Moscow asked the ILRS to end tracking on the satellite,{{Cite web |date=April 19, 2013 |title=BLITS satellite tracking ends - ILRS News |url=https://ilrs.gsfc.nasa.gov/about/news/Past_News.html#2013 |url-status=live |archive-url=https://web.archive.org/web/20240612152853/https://ilrs.gsfc.nasa.gov/about/news/Past_News.html#2013 |archive-date=June 12, 2024 |publisher=International Laser Ranging Service}} because its laser reflector cross section has significantly decreased after the collision, preventing its further use.{{Cite conference |last=Parkhomenko |first=Natalia |last2=Shargorodsky |first2=Victor |last3=Vasiliev |first3=Vladimir |last4=Yurasov |first4=Vasily |date=2013 |title=Accident in orbit |url=https://ilrs.gsfc.nasa.gov/lw18/docs/papers/Posters/13-Po03-Natalia.pdf |conference=18th International Workshop on Laser Ranging |location=Fujiyoshida, Japan |article-number=13-Po03}}

According to the simulation by the Center for Space Standards & Innovation (CSSI), a research arm of Analytical Graphics, Inc. (AGI), BLITS could have been hit by a piece of debris originated by the 2007 Chinese anti-satellite missile test.{{cite web|title= Chinese space debris may have hit Russian satellite|last= Kelso|first= T.S.|date= March 8, 2013|url= http://blogs.agi.com/agi/2013/03/08/chinese-space-debris-hits-russian-satellite/|archive-url= https://web.archive.org/web/20130311041627/http://blogs.agi.com/agi/2013/03/08/chinese-space-debris-hits-russian-satellite/|url-status= dead|archive-date= March 11, 2013|website= AGI Blog|publisher= AGI – Analytical Graphics, Inc.|access-date= February 25, 2014}}

Last science data was returned from the satellite on 5 March 2013.{{cite web|url=https://ilrs.cddis.eosdis.nasa.gov/missions/satellite_missions/past_missions/index.html |title=International Laser Ranging Service |publisher=Ilrs.cddis.eosdis.nasa.gov |date= |accessdate=2022-08-20}}

New version

An improved version of the reflector, named BLITS-M, launched 26 December 2019 with a Gonets-M mission on a Rokot rocket.{{Cite web |last=Krebs |first=Gunter Dirk |title=BLITS-M 1, 2, 3 |url=http://space.skyrocket.de/doc_sdat/blits-m.htm |access-date=7 July 2024 |website=Gunter's Space Page}} BLITS-M failed to separate from the upper stage; thus the mission was a failure.

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References